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1. Experimental Testing of Scattering Polarization Models

2. Frequency Redistribution Function for the Polarized Two-Term Atom

3. Theoretical formulation of Doppler redistribution in scattering polarization within the framework of the velocity-space density matrix formalism

4. Isotropic inelastic and superelastic collisional rates in a multiterm atom

5. Solar magnetism eXplorer (SolmeX)

6. On the Sensitivity of Partial Redistribution Scattering Polarization Profiles to Various Atmospheric Parameters

7. Observations of the Joint Action of the Hanle and Zeeman Effects in the D2 Line of BaII

8. Advanced Forward Modeling and Inversion of Stokes Profiles Resulting from the Joint Action of the Hanle and Zeeman Effects

9. Modelling the incomplete Paschen-Back effect in the spectra of magnetic Ap stars

10. Quiet Sun Magnetic Field Measurements Based on Lines with Hyperfine Structure

11. Standard stars for linear polarization

12. Polarimetric Standardization

13. A Qualitative Interpretation of the Second Solar Spectrum of Ce ll

14. Polynomial Approximants for the Calculation of Polarization Profiles in the \ion{He}{1} 10830 \AA Multiplet

15. Dichroic Masers due to Radiation Anisotropy and the Influence of the Hanle Effect on the Circumstellar SiO Polarization

16. The Hanle and Zeeman Effects in Solar Spicules: A Novel Diagnostic Window on Chromospheric Magnetism

17. Signatures of Incomplete Paschen-Back Splitting in the Polarization Profiles of the He I 10830 multiplet

18. Concerning the existence of a 'turbulent' magnetic field in the quiet Sun

19. On the Atomic Polarization of the Ground Level of Na I

20. Selective Absorption Processes as the Origin of Puzzling Spectral Line Polarization from the Sun

23. Solar magnetism eXplorer (SolmeX): Exploring the magnetic field in the upper atmosphere of our closest star

26. PeNCIL: A Wire Grid Polarimeter at 121.6 nm.

36. Polynomial Approximants for the Calculation of Polarization Profiles in the \ion{He}{1} 10830 ��Multiplet

38. Solar magnetism eXplorer (SolmeX)

40. Astrophysical Plasmas.

44. Spectropolarimetric signatures of anisotropic velocity distributions of optically thin coronal UV lines.

47. Selective absorption processes as the origin of puzzling spectral line polarization from the Sun.

48. Interpretation of second solar spectrum observations of the Sr I 4607 Å line in a quiet region: Turbulent magnetic field strength determination

49. The Zeeman effect: applications to solar physics

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